Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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Naji, M.
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Nozawa, T.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (6/6 displayed)

  • 2016Carbon and silicate dust formation in V1280 Scocitations
  • 2015Evolution of grain size distribution in high-redshift dusty quasars: integrating large amounts of dust and unusual extinction curves.39citations
  • 2014The Origin of the Most Iron-poor Star47citations
  • 2013How do the extinction curves in galaxies evolve?citations
  • 2009Properties of Newly Formed Dust by SN 2006JC Based on Near- to Mid-Infrared Observation With AKARI45citations
  • 2008The Peculiar Type Ib Supernova 2006jc: A WCO Wolf-Rayet Star Explosion50citations

Places of action

Chart of shared publication
Kozasa, T.
3 / 3 shared
Takahashi, H.
1 / 15 shared
Shimonishi, T.
1 / 1 shared
Ohsawa, R.
1 / 1 shared
Oanaka, T.
1 / 1 shared
Sako, S.
1 / 3 shared
Fujiyoshi, T.
1 / 1 shared
Kimura, Y.
1 / 2 shared
Usui, Fumihiko
2 / 4 shared
Koo, B. -C.
1 / 1 shared
Nagayama, T.
1 / 1 shared
Uemura, M.
1 / 1 shared
Arai, A.
1 / 2 shared
Sakon, I.
3 / 3 shared
Asano, R. S.
1 / 2 shared
Takeuchi, T. T.
1 / 4 shared
Chieffi, Alessandro
2 / 7 shared
Limongi, M.
2 / 3 shared
Omukai, K.
1 / 1 shared
Schneider, R.
1 / 39 shared
Yoshida, N.
1 / 1 shared
Marassi, S.
1 / 1 shared
Chiaki, G.
1 / 1 shared
Takeuchi, T.
1 / 6 shared
Asano, R.
1 / 1 shared
Kaneda, H.
2 / 4 shared
Minezaki, T.
2 / 4 shared
Nakagawa, T.
1 / 2 shared
Umeda, H.
1 / 1 shared
Ohyabu, S.
1 / 1 shared
Ishihara, D.
1 / 2 shared
Matsuhara, H.
1 / 1 shared
Yoshii, Y.
2 / 4 shared
Wada, T.
2 / 9 shared
Nomoto, K.
2 / 2 shared
Tanabé, T.
2 / 2 shared
Tominaga, N.
2 / 2 shared
Ohyama, Y.
2 / 2 shared
Tanaka, M.
2 / 18 shared
Onaka, T.
2 / 2 shared
Suzuki, T.
2 / 19 shared
Murakami, H.
1 / 5 shared
Gurugubelli, U. K.
1 / 1 shared
Sahu, D. K.
1 / 1 shared
Deng, J.
1 / 4 shared
Anupama, G. C.
1 / 1 shared
Kawabata, K. S.
1 / 1 shared
Maeda, K.
1 / 4 shared
Prabhu, T. P.
1 / 1 shared
Tornambe, A.
1 / 1 shared
Chart of publication period
2016
2015
2014
2013
2009
2008

Co-Authors (by relevance)

  • Kozasa, T.
  • Takahashi, H.
  • Shimonishi, T.
  • Ohsawa, R.
  • Oanaka, T.
  • Sako, S.
  • Fujiyoshi, T.
  • Kimura, Y.
  • Usui, Fumihiko
  • Koo, B. -C.
  • Nagayama, T.
  • Uemura, M.
  • Arai, A.
  • Sakon, I.
  • Asano, R. S.
  • Takeuchi, T. T.
  • Chieffi, Alessandro
  • Limongi, M.
  • Omukai, K.
  • Schneider, R.
  • Yoshida, N.
  • Marassi, S.
  • Chiaki, G.
  • Takeuchi, T.
  • Asano, R.
  • Kaneda, H.
  • Minezaki, T.
  • Nakagawa, T.
  • Umeda, H.
  • Ohyabu, S.
  • Ishihara, D.
  • Matsuhara, H.
  • Yoshii, Y.
  • Wada, T.
  • Nomoto, K.
  • Tanabé, T.
  • Tominaga, N.
  • Ohyama, Y.
  • Tanaka, M.
  • Onaka, T.
  • Suzuki, T.
  • Murakami, H.
  • Gurugubelli, U. K.
  • Sahu, D. K.
  • Deng, J.
  • Anupama, G. C.
  • Kawabata, K. S.
  • Maeda, K.
  • Prabhu, T. P.
  • Tornambe, A.
OrganizationsLocationPeople

document

Carbon and silicate dust formation in V1280 Sco

  • Kozasa, T.
  • Takahashi, H.
  • Shimonishi, T.
  • Ohsawa, R.
  • Oanaka, T.
  • Sako, S.
  • Fujiyoshi, T.
  • Kimura, Y.
  • Usui, Fumihiko
  • Nozawa, T.
  • Koo, B. -C.
  • Nagayama, T.
  • Uemura, M.
  • Arai, A.
  • Sakon, I.
Abstract

This study investigates the temporal evolution of the infrared emission from the dusty nova V1280 Sco over 2000 days from the outburst. We have revealed that the infrared spectral energy distributions at 1272, 1616 and 1947 days are explained by the emissions produced by amorphous carbon dust of mass (6.6-8.7) × 10<SUP>-8</SUP> M<SUB>ʘ</SUB> with a representative grain size of 0.01 µm and astronomical silicate dust of mass (3.4-4.3) × 10<SUP>-7</SUP> M<SUB>ʘ</SUB> with a representative grain size of 0.3-0.5 µm. Both of carbon and silicate dust travel farther away from the white dwarf without an apparent mass evolution throughout those later epochs....

Topics
  • amorphous
  • Carbon
  • grain
  • grain size